The excellent throughput and low background rates of FUSE
enable observations of many dozens of AGN at wavelengths
shortward of 1200 Å. Early FUSE observations of AGN
include ESO141--G55, PG0052+251, PG0804+761, VII Zw 118,
H1821+64, Mrk 352, Mrk 876, and HS 1700+64. In
contemporaneous observing programs, we are also obtaining
longer-wavelength UV spectra with HST/STIS covering
1150--3200 Å, and ground-based spectra from the
atmospheric limit to 1 \mum, for many of the FUSE program
objects. We will discuss the intrinsic properties of the
observed AGN and show sample spectral energy distributions
covering the 912--10,000 Å\ observed wavelength range.

This work is supported by NASA contract NAS5-32985.

The author(s) of this abstract have provided an email address
for comments about the abstract:
gak@stsci.edu